Saros Series of Lunar Eclipses

Lunar Eclipses in Saros Series 133

This page lists all the lunar eclipses in saros series 133. The series contains 71 eclipses, occurring over 1262 years.

The following chart shows the position where the Moon
is directly overhead at the maximum times of the
total (in blue) and
partial (in red) lunar eclipses (penumbral eclipses are
omitted). Each eclipse will be visible approximately
from the half of the Earth centred on that point. Note
that we only have mapping data for
eclipses from year 1 AD, so any eclipses prior to that
date will be missing. Use the
zoom controls on the left to zoom in and out; hover over
a marker to see the area of visibility and summary
information on that eclipse.

Enable JavaScript to see the interactive map.

Note that eclipse dates are specified relative to UT.
You have not selected a timezone for eclipse timings, so all times are shown in UT (essentially GMT).

In this extremely marginal eclipse, the Moon barely clipped the edge of the Earth's penumbral shadow. This caused a microscopic darkening of just 7% of the Moon's disc for 1 hour and 24 minutes, which was essentially impossible to see.

This very subtle penumbral eclipse eclipse was essentially invisible to the naked eye; though it lasted 2 hours and 24 minutes, just 22% of the Moon's disc was in partial shadow (with no part of it in complete shadow).

This very subtle penumbral eclipse eclipse was essentially invisible to the naked eye; though it lasted 3 hours and 4 minutes, just 38% of the Moon's disc was in partial shadow (with no part of it in complete shadow).

This very subtle penumbral eclipse eclipse was essentially invisible to the naked eye; though it lasted 3 hours and 36 minutes, just 54% of the Moon's disc was in partial shadow (with no part of it in complete shadow).

This subtle penumbral eclipse eclipse may have been visible to a skilled observer at maximum eclipse. 69% of the Moon's disc was partially shaded by the Earth (none of it was in total shadow), which caused a gentle shadow gradient across its disc at maximum; the eclipse as a whole lasted 4 hours and 2 minutes.

This subtle penumbral eclipse eclipse may have been visible to a skilled observer at maximum eclipse. 85% of the Moon's disc was partially shaded by the Earth (none of it was in total shadow), which caused a gentle shadow gradient across its disc at maximum; the eclipse as a whole lasted 4 hours and 23 minutes.

In a rare total penumbral eclipse, the entire Moon was partially shaded by the Earth (though none of it was in complete shadow), and the shading across the Moon should have been quite visible at maximum eclipse. The penumbral phase lasted for 4 hours and 41 minutes in all, though for most of it, the eclipse was extremely difficult or impossible to see.

A tiny bite out of the Moon may have been visible at maximum, though just 9% of the Moon was shadowed in a partial eclipse which lasted for 1 hour and 14 minutes. A shading across the moon from the Earth's penumbral shadow should have been visible at maximum eclipse.

The Moon was almost covered by the Earth's shadow in a very deep partial eclipse, which lasted 3 hours and 19 minutes. With 92% of the Moon in shadow at maximum eclipse, this was quite a memorable event.

The Moon was almost covered by the Earth's shadow in a very deep partial eclipse, which lasted 3 hours and 20 minutes. With 95% of the Moon in shadow at maximum eclipse, this was quite a memorable event.

The Moon was almost covered by the Earth's shadow in a very deep partial eclipse, which lasted 3 hours and 21 minutes. With 98% of the Moon in shadow at maximum eclipse, this was quite a memorable event.

The Moon was almost covered by the Earth's shadow in a very deep partial eclipse, which lasted 3 hours and 22 minutes. With 99% of the Moon in shadow at maximum eclipse, this was quite a memorable event.

The Moon barely edged into total eclipse for just 12 minutes exactly. With the Moon just barely inside the Earth's umbral shadow, the Moon may have been quite bright, but even so, this should have been worth seeing. The partial eclipse lasted for 3 hours and 22 minutes in total.

The Moon barely edged into total eclipse for 20 minutes and 48 seconds. With the Moon just 2% of its diameter into the Earth's umbral shadow, the Moon may have been quite bright, but even so, this should have been worth seeing. The partial eclipse lasted for 3 hours and 23 minutes in total.

The Moon barely edged into total eclipse for 28 minutes and 12 seconds. With the Moon just 3% of its diameter into the Earth's umbral shadow, the Moon may have been quite bright, but even so, this should have been worth seeing. The partial eclipse lasted for 3 hours and 23 minutes in total.

The Moon barely edged into total eclipse for 34 minutes and 48 seconds. With the Moon just 5% of its diameter into the Earth's umbral shadow, the Moon may have been quite bright, but even so, this should have been worth seeing. The partial eclipse lasted for 3 hours and 23 minutes in total.

A shallow total eclipse saw the Moon in relative darkness for 42 minutes and 18 seconds. The Moon was 8% of its diameter into the Earth's umbral shadow, and should have been significantly darkened. The partial eclipse lasted for 3 hours and 24 minutes in total.

A shallow total eclipse saw the Moon in relative darkness for 49 minutes and 48 seconds. The Moon was 11% of its diameter into the Earth's umbral shadow, and should have been significantly darkened for viewers over the Americas, Europe, Africa, and western Asia. The partial eclipse lasted for 3 hours and 25 minutes in total.

A shallow total eclipse will see the Moon in relative darkness for 58 minutes and 18 seconds. The Moon will be 15% of its diameter into the Earth's umbral shadow, and should be significantly darkened for viewers in east Asia, Australia, North America, and Central America. The partial eclipse will last for 3 hours and 27 minutes in total.

The Moon will be plunged into darkness for 1 hour and 6 minutes, in a deep total eclipse which will see the Moon 20% of its diameter inside the Earth's umbral shadow. The visual effect of this depends on the state of the Earth's atmosphere, but the Moon may be stained a deep red colour. The partial eclipse will last for 3 hours and 29 minutes in total.

The Moon will be plunged into darkness for 1 hour and 15 minutes, in a deep total eclipse which will see the Moon 27% of its diameter inside the Earth's umbral shadow. The visual effect of this depends on the state of the Earth's atmosphere, but the Moon may be stained a deep red colour. The partial eclipse will last for 3 hours and 31 minutes in total.

The Moon will be plunged into darkness for 1 hour and 22 minutes, in a deep total eclipse which will see the Moon 35% of its diameter inside the Earth's umbral shadow. The visual effect of this depends on the state of the Earth's atmosphere, but the Moon may be stained a deep red colour. The partial eclipse will last for 3 hours and 34 minutes in total.

The Moon will be plunged into darkness for 1 hour and 29 minutes, in a deep total eclipse which will see the Moon 44% of its diameter inside the Earth's umbral shadow. The visual effect of this depends on the state of the Earth's atmosphere, but the Moon may be stained a deep red colour. The partial eclipse will last for 3 hours and 36 minutes in total.

The Moon will be plunged into darkness for 1 hour and 35 minutes, in a deep total eclipse which will see the Moon 54% of its diameter inside the Earth's umbral shadow. The visual effect of this depends on the state of the Earth's atmosphere, but the Moon may be stained a deep red colour. The partial eclipse will last for 3 hours and 38 minutes in total.

A dramatic total eclipse lasting 1 hour and 39 minutes will plunge the full Moon into deep darkness, as it passes right through the centre of the Earth's umbral shadow. While the visual effect of a total eclipse is variable, the Moon may be stained a deep orange or red colour at maximum eclipse. This will be a great spectacle for everyone who sees it. The partial eclipse will last for 3 hours and 39 minutes in total.

A dramatic total eclipse lasting 1 hour and 41 minutes will plunge the full Moon into deep darkness, as it passes right through the centre of the Earth's umbral shadow. While the visual effect of a total eclipse is variable, the Moon may be stained a deep orange or red colour at maximum eclipse. This will be a great spectacle for everyone who sees it. The partial eclipse will last for 3 hours and 40 minutes in total.

A dramatic total eclipse lasting 1 hour and 42 minutes will plunge the full Moon into deep darkness, as it passes right through the centre of the Earth's umbral shadow. While the visual effect of a total eclipse is variable, the Moon may be stained a deep orange or red colour at maximum eclipse. This will be a great spectacle for everyone who sees it. The partial eclipse will last for 3 hours and 39 minutes in total.

A dramatic total eclipse lasting 1 hour and 40 minutes will plunge the full Moon into deep darkness, as it passes right through the centre of the Earth's umbral shadow. While the visual effect of a total eclipse is variable, the Moon may be stained a deep orange or red colour at maximum eclipse. This will be a great spectacle for everyone who sees it. The partial eclipse will last for 3 hours and 38 minutes in total.

The Moon will be plunged into darkness for 1 hour and 35 minutes, in a deep total eclipse which will see the Moon 57% of its diameter inside the Earth's umbral shadow. The visual effect of this depends on the state of the Earth's atmosphere, but the Moon may be stained a deep red colour. The partial eclipse will last for 3 hours and 36 minutes in total.

The Moon will be plunged into darkness for 1 hour and 28 minutes, in a deep total eclipse which will see the Moon 43% of its diameter inside the Earth's umbral shadow. The visual effect of this depends on the state of the Earth's atmosphere, but the Moon may be stained a deep red colour. The partial eclipse will last for 3 hours and 32 minutes in total.

The Moon will be plunged into darkness for 1 hour and 16 minutes, in a deep total eclipse which will see the Moon 30% of its diameter inside the Earth's umbral shadow. The visual effect of this depends on the state of the Earth's atmosphere, but the Moon may be stained a deep red colour. The partial eclipse will last for 3 hours and 27 minutes in total.

A shallow total eclipse will see the Moon in relative darkness for 59 minutes exactly. The Moon will be 16% of its diameter into the Earth's umbral shadow, and should be significantly darkened. The partial eclipse will last for 3 hours and 21 minutes in total.

The Moon will barely edge into total eclipse for 27 minutes and 6 seconds. With the Moon just 3% of its diameter into the Earth's umbral shadow, the Moon may be quite bright, but even so, this should be worth seeing. The partial eclipse will last for 3 hours and 13 minutes in total.

The Moon will be almost covered by the Earth's shadow in a very deep partial eclipse, lasting 3 hours and 5 minutes. With 91% of the Moon in shadow at maximum eclipse, this will be quite a memorable event.

A tiny bite out of the Moon may be visible at maximum, though just 10% of the Moon will be shadowed in a partial eclipse lasting for 1 hour and 7 minutes. A shading across the moon from the Earth's penumbral shadow should be visible at maximum eclipse.

A tiny bite out of the Moon may be visible at maximum, though just 7% of the Moon will be shadowed in a partial eclipse lasting for 58 minutes and 36 seconds. A shading across the moon from the Earth's penumbral shadow should be visible at maximum eclipse.

A tiny bite out of the Moon may be visible at maximum, though just 4% of the Moon will be shadowed in a partial eclipse lasting for 44 minutes and 12 seconds. A shading across the moon from the Earth's penumbral shadow should be visible at maximum eclipse.

The Moon will approach within 0% of the Earth's umbral shadow at maximum eclipse, with the overall eclipse lasting 3 hours and 59 minutes. While less dramatic than a partial eclipse (as no part of the Moon will be in complete shadow), a shading across the Moon should be readily visible to observers.

At maximum eclipse, 90% of the Moon's disc will be partially shaded by the Earth, which will cause a slight shadow gradient across its disc; this subtle effect may be visible to careful observers. No part of the Moon will be in complete shadow. The eclipse will last 3 hours and 53 minutes overall.

At maximum eclipse, 84% of the Moon's disc will be partially shaded by the Earth, which will cause a slight shadow gradient across its disc; this subtle effect may be visible to careful observers. No part of the Moon will be in complete shadow. The eclipse will last 3 hours and 46 minutes overall.

This subtle penumbral eclipse eclipse may be visible to a skilled observer at maximum eclipse. 76% of the Moon's disc will be partially shaded by the Earth (none of it will be in total shadow), which will cause a gentle shadow gradient across its disc at maximum; the eclipse as a whole will last 3 hours and 37 minutes.

This subtle penumbral eclipse eclipse may be visible to a skilled observer at maximum eclipse. 67% of the Moon's disc will be partially shaded by the Earth (none of it will be in total shadow), which will cause a gentle shadow gradient across its disc at maximum; the eclipse as a whole will last 3 hours and 26 minutes.

This very subtle penumbral eclipse eclipse will be essentially invisible to the naked eye; though it will last 3 hours and 11 minutes, just 57% of the Moon's disc will be in partial shadow (with no part of it in complete shadow).

This very subtle penumbral eclipse eclipse will be essentially invisible to the naked eye; though it will last 2 hours and 54 minutes, just 46% of the Moon's disc will be in partial shadow (with no part of it in complete shadow).

This very subtle penumbral eclipse eclipse will be essentially invisible to the naked eye; though it will last 2 hours and 32 minutes, just 34% of the Moon's disc will be in partial shadow (with no part of it in complete shadow).

This very subtle penumbral eclipse eclipse will be essentially invisible to the naked eye; though it will last 2 hours and 2 minutes, just 21% of the Moon's disc will be in partial shadow (with no part of it in complete shadow).

In this extremely marginal eclipse, the Moon barely clips the edge of the Earth's penumbral shadow. This will cause a microscopic darkening of just 9% of the Moon's disc for 1 hour and 18 minutes, which will be essentially impossible to see.